Constant-roll approach has opened a new window to analyze cosmic inflation due to the consideration of a constant rate of rolling for inflaton. The model is becoming very popular since a wide range of inflationary models has been investigated in the context of constant-roll inflation [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}, [9]}, [10]}, [11]}, [12]}, [13]}, [14]}, [15]}, [16]}, [17]}, [18]}, [19]}. In the present manuscript, we study a fermionic inflationary model in which a fermionic field which is non-minimally coupled to gravity is the main responsible to drive inflation instead of inflaton introduced in the standard inflationary paradigm. In fact, Noether symmetry arguments of the model show an exponentially expanding universe if a non-minimal coupling between the fermionic field and the Ricci scalar is considered [20]}. Fermionic fields also are known as gravitational sources of dark energy as the late-time accelerating of the universe in addition to playing the role of inflaton for the early time acceleration [21]}. Moreover, the interaction of a fermionic field with a scalar field can be recognized as the source of interacting dark
matter-dark energy [22]}. Such theories that deal with fermionic fields instead of scalar fields are named the Fermions Tensor Theories (FTT) [23]}, [24]}, [25]}, [26]}.
